The second data release of the Sloan Digital Sky Survey

被引:1013
作者
Abazajian, K
Adelman-McCarthy, JK
Agüeros, MA
Allam, SS
Kurt
Anderson, SJ
Anderson, SF
Annis, J
Bahcall, NA
Baldry, IK
Bastian, S
Berlind, A
Bernardi, M
Blanton, MR
Bochanski, JJ
Boroski, WN
Briggs, JW
Brinkmann, J
Brunner, RJ
Budavári, T
Carey, LN
Carliles, S
Castander, FJ
Connolly, AJ
Csabai, I
Doi, M
Dong, F
Eisenstein, DJ
Evans, ML
Fan, XH
Finkbeiner, DP
Friedman, SD
Frieman, JA
Fukugita, M
Gal, RR
Gillespie, B
Glazebrook, K
Gray, J
Grebel, EK
Gunn, JE
Gurbani, VK
Hall, PB
Hamabe, M
Harris, FH
Harris, HC
Harvanek, M
Heckman, TM
Hendry, JS
Hennessy, GS
Hindsley, RB
机构
[1] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA
[2] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[3] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[4] New Mexico State Univ, Dept Astron, MSC 4500, Las Cruces, NM 88003 USA
[5] Apache Point Observ, Sunspot, NM 88349 USA
[6] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[7] Johns Hopkins Univ, Dept Phys & Astron, Ctr Astrophys Sci, Baltimore, MD 21218 USA
[8] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[9] Univ Chicago, Ctr Cosmol Phys, Chicago, IL 60637 USA
[10] NYU, Dept Phys, Ctr Cosmol & Particle Phys, New York, NY 10003 USA
[11] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA
[12] Univ Illinois, Dept Astron, Urbana, IL 61801 USA
[13] CSIC, Inst Estudis Espacials Catalunya, E-08034 Barcelona, Spain
[14] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA
[15] Eotvos Lorand Univ, Dept Phys Complex Syst, H-1518 Budapest, Hungary
[16] Univ Tokyo, Sch Sci, Inst Astron, Tokyo 1810015, Japan
[17] Univ Tokyo, Sch Sci, Res Ctr Early Universe, Tokyo 1810015, Japan
[18] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[19] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[20] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
[21] Microsoft Res, San Francisco, CA 94105 USA
[22] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[23] Lucent Technol, Naperville, IL 60566 USA
[24] Japan Womens Univ, Dept Math & Phys Sci, Bunkyo Ku, Tokyo 1128681, Japan
[25] USN Observ, Flagstaff Stn, Flagstaff, AZ 86002 USA
[26] USN Observ, Washington, DC 20392 USA
[27] USN, Remote Sensing Div, Res Lab, Washington, DC 20392 USA
[28] Natl Astron Observ, Tokyo 1818588, Japan
[29] Tohoku Univ, Astron Inst, Aoba Ku, Sendai, Miyagi 9808578, Japan
[30] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[31] Akad Pedag Krakowie, Obserwatorium Astron Suhorze, PL-30084 Krakow, Poland
[32] CERN, IT Div, CH-1211 Geneva 23, Switzerland
[33] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA
[34] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA
[35] Univ Colorado, Ctr Astrophys & Space Astron, Boulder, CO 80309 USA
[36] Univ Sussex, Ctr Astron, Brighton BN1 9QJ, E Sussex, England
[37] Nagoya Univ, Dept Phys & Astrophys, Chikusa Ku, Nagoya, Aichi 4648602, Japan
[38] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[39] Univ Edinburgh, Royal Observ, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
[40] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA
[41] Rensselaer Polytech Inst, Dept Phys Appl Phys & Astron, Troy, NY 12180 USA
[42] CMC Elect Aurora, Sugar Grove, IL 60554 USA
[43] Univ Tokyo, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
[44] Univ Tokyo, Res Ctr Early Universe, Bunkyo Ku, Tokyo 1130033, Japan
[45] Princeton Univ, Joseph Henry Labs, Princeton, NJ 08544 USA
[46] Rochester Inst Technol, Dept Phys, Rochester, NY 14623 USA
[47] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA
[48] Univ Tokyo, Inst Cosm Ray Res, Japan Participat Grp, Kashiwa, Chiba 2778582, Japan
[49] Univ Zagreb, Dept Phys, Zagreb 10000, Croatia
[50] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
关键词
atlases; catalogs; surveys;
D O I
10.1086/421365
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second Data Release. This data release consists of 3324 deg(2) of five-band (ugriz) imaging data with photometry for over 88 million unique objects, 367,360 spectra of galaxies, quasars, stars, and calibrating blank sky patches selected over 2627 deg(2) of this area, and tables of measured parameters from these data. The imaging data reach a depth of r approximate to 22.2 ( 95% completeness limit for point sources) and are photometrically and astrometrically calibrated to 2% rms and 100 mas rms per coordinate, respectively. The imaging data have all been processed through a new version of the SDSS imaging pipeline, in which the most important improvement since the last data release is fixing an error in the model fits to each object. The result is that model magnitudes are now a good proxy for point-spread function magnitudes for point sources, and Petrosian magnitudes for extended sources. The spectroscopy extends from 3800 to 9200 8 at a resolution of 2000. The spectroscopic software now repairs a systematic error in the radial velocities of certain types of stars and has substantially improved spectrophotometry. All data included in the SDSS Early Data Release and First Data Release are reprocessed with the improved pipelines and included in the Second Data Release. Further characteristics of the data are described, as are the data products themselves and the tools for accessing them.
引用
收藏
页码:502 / 512
页数:11
相关论文
共 41 条
[1]  
ABAZAJIAN K, 2003, AJ, V126, P2018
[2]   An efficient targeting strategy for multiobject spectrograph surveys: The Sloan Digital Sky Survey "tiling'' algorithm [J].
Blanton, MR ;
Lin, H ;
Lupton, RH ;
Maley, FM ;
Young, N ;
Zehavi, I ;
Loveday, J .
ASTRONOMICAL JOURNAL, 2003, 125 (04) :2276-2286
[3]   Spectrophotometric standards from the far-ultraviolet to the near-infrared: STIS and NICMOS fluxes [J].
Bohlin, RC ;
Dickinson, ME ;
Calzetti, D .
ASTRONOMICAL JOURNAL, 2001, 122 (04) :2118-2128
[4]  
DOI M, 2004, UNPUB
[5]   Spectroscopic target selection for the Sloan Digital Sky Survey: The luminous red galaxy sample [J].
Eisenstein, DJ ;
Annis, J ;
Gunn, JE ;
Szalay, AS ;
Connolly, AJ ;
Nichol, RC ;
Bahcall, NA ;
Bernardi, M ;
Burles, S ;
Castander, FJ ;
Fukugita, M ;
Hogg, DW ;
Ivezic, Z ;
Knapp, GR ;
Lupton, RH ;
Narayanan, V ;
Postman, M ;
Reichart, DE ;
Richmond, M ;
Schneider, DP ;
Schlegel, DJ ;
Strauss, MA ;
SubbaRao, M ;
Tucker, DL ;
Vanden Berk, D ;
Vogeley, MS ;
Weinberg, DH ;
Yanny, B .
ASTRONOMICAL JOURNAL, 2001, 122 (05) :2267-2280
[6]   The temperature scale and mass distribution of hot DA white dwarfs [J].
Finley, DS ;
Koester, D ;
Basri, G .
ASTROPHYSICAL JOURNAL, 1997, 488 (01) :375-396
[7]   The Sloan digital sky survey photometric system [J].
Fukugita, M ;
Ichikawa, T ;
Gunn, JE ;
Doi, M ;
Shimasaku, K ;
Schneider, DP .
ASTRONOMICAL JOURNAL, 1996, 111 (04) :1748-1756
[8]   Automatic redshift determination by use of principal component analysis. I. Fundamentals [J].
Glazebrook, K ;
Offer, AR ;
Deeley, K .
ASTROPHYSICAL JOURNAL, 1998, 492 (01) :98-109
[9]   Proper-motion catalog from SDSS ∧ USNO-B [J].
Gould, A ;
Kollmeier, JA .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2004, 152 (01) :103-111
[10]   THE CALIBRATION OF MK SPECTRAL CLASSES USING SPECTRAL-SYNTHESIS .1. THE EFFECTIVE TEMPERATURE CALIBRATION OF DWARF STARS [J].
GRAY, RO ;
CORBALLY, CJ .
ASTRONOMICAL JOURNAL, 1994, 107 (02) :742-746